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Community shelf Community shelf -> All the Reactions, you kneed to know for IITJEE(actually,quiet more)..in this article..... -> Go to message
This Post 5 points    (Olaaa!! Perrrfect answer.   in 1 votes )   [?]
1 replies   




















Hey guys , here is a list of all the name reactions possible in IITJEE.

Click on any one to view mechanism................

Good rates and comments expected................ 


a











b



















c



















d











e







f












g







h















i



j




k









l




m












n







o






p

















q

r









s























t






u




v


w














x

y


z

 

 

jst click on ne to see it




Catalogs Discussion Forums -> General -> Hey guys! Let's start a great game ...... -> Go to message
This Post 2 points    (Olaaa!! Perrrfect answer.   in 1 votes )   [?]
102 replies   

Hey man,plz don't expect rates before u have rated others........

Catalogs Discussion Forums -> General -> Hey guys! Let's start a great game ...... -> Go to message
This Post 0 points    (Olaaa!! Perrrfect answer.   in 0 votes )   [?]
102 replies   

Stereoisomers made easy:...


1.in non symmetric molecules with n chiral atoms:2^n.


2.in symmetric molecules with n(even) chiral atoms:2^(n-1).


3.in symmetric molecules with n(odd) chiral atoms:2^(n-1)-2^(n/2-1/2).


VERY HELPFUL....

Community shelf Community shelf -> Do you know how the schrodinger wave equation was derived???? -> Go to message
This Post 0 points    (Olaaa!! Perrrfect answer.   in 0 votes )   [?]
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Come on ppl...................................
Catalogs Discussion Forums -> General -> Hey guys! Let's start a great game ...... -> Go to message
This Post 2 points    (Olaaa!! Perrrfect answer.   in 1 votes )   [?]
102 replies   

 


1.P=h(rho)g


2.cosa+isina=e^ia

Community shelf Community shelf -> Do you know how the schrodinger wave equation was derived???? -> Go to message
This Post 25 points    (Olaaa!! Perrrfect answer.   in 5 votes )   [?]
3 replies   


SCHRODINGER WAVE EQUATION DERIVATION:



 



 



                                         



  Schrödinger's equation follows very naturally      earlier developments:



In 1905, by considering the photoelectric effect, Albert Einstein had published his



E = h f\;


formula for the relation between the energy E and frequency f of the quanta of radiation (photons), where h is Planck's constant.



In 1924 Louis de Broglie presented his de Broglie hypothesis which states that all particles (not just photons) have an associated wavefunction \Psi\; with properties:



p=h / \lambda\;, where \lambda\, is the wavelength of the wave and p the momentum of the particle.


De Broglie showed that this was consistent with Einstein's formula and special relativity so that



E = h f\;


still holds, but now this is hypothesized to hold for all particles, not just photons anymore.



Expressed in terms of angular frequency \omega = 2\pi f\; and wavenumber k = 2\pi / \lambda\;, with \hbar = h / 2 \pi\; we get:



E=\hbar \omega


and



\mathbf{p}=\hbar \mathbf{k}\;


where we have expressed p and k as vectors.



Schrödinger's great insight, late in 1925, was to express the phase of a plane wave as a complex phase factor:



\psi \approx e^{i(\mathbf{k}\cdot\mathbf{x}- \omega t)}


and to realize that since



 \frac{\partial}{\partial t} \psi = -i\omega \psi


then



 E \psi = \hbar \omega \psi =  i\hbar\frac{\partial}{\partial t} \psi


and similarly since:



 \frac{\partial}{\partial x} \psi = i k_x \psi


then



 p_x \psi = \hbar k_x \psi = -i\hbar\frac{\partial}{\partial x} \psi


and hence:



 p_x^2 \psi = -\hbar^2\frac{\partial^2}{\partial x^2} \psi


so that, again for a plane wave, he got:



 p^2 \psi = (p_x^2 + p_y^2 + p_z^2) \psi = -\hbar^2\left(\frac{\partial^2}{\partial x^2} + \frac{\partial^2}{\partial y^2} + \frac{\partial^2}{\partial z^2}\right) \psi = -\hbar^2\nabla^2 \psi


And by inserting these expressions into the Newtonian formula for a particle with total energy E, mass m, moving in a potential V:



E=\frac{p^2}{2m}+V (simply the sum of the kinetic energy and potential energy; the plane wave model assumed V = 0)


he got his famed equation for a single particle in the 3-dimensional case in the presence of a potential:



i\hbar\frac{\partial}{\partial t}\Psi=-\frac{\hbar^2}{2m}\nabla^2\Psi + V\Psi


Using this equation, Schrödinger computed the spectral lines for hydrogen by treating a hydrogen atom's single negatively charged electron as a wave, \psi\;, moving in a potential well, V, created by the positively charged proton. This computation tallied with experiment, the Bohr model and also the results of Werner Heisenberg's matrix mechanics - but without having to introduce Heisenberg's concept of non-commuting observables. Schrödinger published his wave equation and the spectral analysis of hydrogen in a series of four papers in 1926.



The Schrödinger equation defines the behaviour of \psi\;, but does not interpret what \psi\; is. Schrödinger tried unsuccessfully to interpret it as a charge density. In 1926 Max Born, just a few days after Schrödinger's fourth and final paper was published, successfully interpreted \psi\; as a probability amplitude, although Schrödinger was never reconciled to this statistical or probabilistic approach.



 



In the mathematical formulation of quantum mechanics, a physical system is associated with a complex Hilbert space such that each instantaneous state of the system is described by a ray in that space. The nonzero elements of a Hilbert space are by definition normalizable and it is convenient, although not necessary, to represent a state by an element of the ray which is normalized to unity. This vector is often somewhat loosely referred to as wave function, although in a more rigorous formulation of quantum mechanics a wave function is a special case of a state vector. (In fact, a wave function is a state in the position representation, see below). A state vector encodes the probabilities for the outcomes of all possible measurements applied to the system. It contains all information of the system that is knowable in a quantum mechanical sense. As the state of a system generally changes over time, the state vector is a function of time. The Schrödinger equation provides a quantitative description of the rate of change of the state vector.



In Dirac's bra-ket notation at time t the state is given by the ket |\psi(t)\rangle. The time-dependent Schrödinger equation, giving the time evolution of the ket, is:



H(t)\left|\psi\left(t\right)\right\rangle = \mathrm{i}\hbar \frac{d}{d t} \left| \psi \left(t\right) \right\rangle


where i is the imaginary unit, t is time, d / dt is the derivative with respect to t, \hbar is the reduced Planck's constant (Planck's constant divided by 2\pi\,), \psi(t)\, is the time dependent state vector, and H(t) is the Hamiltonian (a self-adjoint operator acting on the state space). If one assumes a certain representation for \psi\,, for instance position or momentum representation, the state vector is assumed to depend on more variables than time alone, and the time derivative must be replaced by the partial derivative \partial / \partial t.



The Hamiltonian describes the total energy of the system. As with the force occurring in Newton's second law, its form is not provided by the Schrödinger equation, but must be independently determined from the physical properties of the system.



 



                                   



 


GOOD RATES EXPECTED<\.....


Community shelf Community shelf -> DO YOU KNOW THE SUN VERY WELL????? THINK AGAIN!!!! -> Go to message
This Post 0 points    (Olaaa!! Perrrfect answer.   in 0 votes )   [?]
4 replies   
some one plz comment!!
Community shelf Community shelf -> DO YOU KNOW THE SUN VERY WELL????? THINK AGAIN!!!! -> Go to message
This Post 11 points    (Olaaa!! Perrrfect answer.   in 4 votes )   [?]
4 replies   

PHASES OF A STAR:

heavenly bodies in your not-so-friendly galactic neighbourhood.............

Beware,in a few 100 million years ,our fate could rest upon one of these , with our own friendly sun,turning on full-throttle against us....................................

Read on...........

 

 

Evolution of stars
The life cycles of stars follow three general patterns, each associated with a range of initial mass. There are (1) high-mass stars, which have more than 8 solar masses; (2) intermediate-mass stars, with 0.5 to 8 solar masses -- the group that includes the sun; and (3) low-mass stars, with 0.1 to 0.5 solar mass. Objects with less than 0.1 solar mass do not have enough gravitational force to produce the core temperature necessary for hydrogen fusion.
The life cycles of single stars are simpler than those of binary systems, so this section discusses the evolution of single stars first. And because astronomers know much more about the sun than any other star, the discussion begins with the development of intermediate-mass stars.

 

Image:CMB Timeline75.jpg

 

our sun now:


 

But a few million years from now:..........

It could: ..............................................

 

 become a Main Phase Star

 

 become a Red giant star

 

 become an Asymptotic Giant star

 

  become A white dwarf star

 

  become A black dwarf star

 

 undergo a supernova

 

 become a neutron star

 

 become a magnetar

 

 become a quasar..

 


 

Or the most dangerous of all a massive star devouring black hole....................

 

After reading this you certainly would'nt want to live at that time......................

Think about it........

 

Good Rates Expected.....



Catalogs Discussion Forums -> General -> Hey guys! Let's start a great game ...... -> Go to message
This Post 10 points    (Olaaa!! Perrrfect answer.   in 2 votes )   [?]
102 replies   

Hey guys remember to vote for the person with maximum pts.


formulae:


E=-dv/dr....


F=I.dlXB...

Catalogs Discussion Forums -> General -> Fire ,fire eveywhere!!!! -> Go to message
This Post 0 points    (Olaaa!! Perrrfect answer.   in 0 votes )   [?]
0 replies   

Hey guys ,check out the great article on fire below!! Ever wondered wat fire was??? You will have your answers  cleared now...


BE sure to rate and comment for improvement.....

Community shelf Community shelf -> Fire,fire everywhere? But no questions answered?? THINK AGAIN!! -> Go to message
This Post 0 points    (Olaaa!! Perrrfect answer.   in 0 votes )   [?]
2 replies   
please comment guys?
Community shelf Community shelf -> Fire,fire everywhere? But no questions answered?? THINK AGAIN!! -> Go to message
This Post 9 points    (Olaaa!! Perrrfect answer.   in 3 votes )   [?]
2 replies   


What exactly is fire? Is it purely energy? What state of matter is it? Can it be ionized? Can it be affected by magnetism? Gravity?








Confused,..well first think read the theory and then check for yourselves...








The correct definition needed to understand fire's properties is:








"Fire is the rapid combination of oxygen with fuel in the presence of heat, typically characterized by flame, a body of incandescent gas that contains and sustains the reaction and emits light and heat."



 











1) Rapid combination of oxygen with fuel in the presence of heat.Oxygen, fuel, and heat are the essential ingredients of fire. 




(2) Typically characterized by flame.  "Typically" allows mus to sidestep the issue of apparently nonflaming fires, like you get with burning charcoal. But charcoal fires do create flame--we just can't see it due to the lack of impurities or incompletely burned fuel in the plume. (we can't see a fuel fire at an Indy or CART race either, because the cars run on clean-burning methanol.) 




(3) Body of incandescent gas. Flame defined. Most encyclopedia and dictionary definitions blow past this entirely, allowing persons such as yourself to imagine that fire is "pure energy" or similar nonsense. We say "body" because the gas has a characteristic structure and composition. We say "incandescent" because (a) it sounds scientific, (b) it means "luminous with intense heat," precisely what we are attempting to convey. 




4) Contains and sustains the reaction. Flame isn't just the result of fire; it is the fire. What's more, without the flame's heat the fire would go out.




(5) Emits light and heat. Duh. However, we mustn't overlook the obvious.











Now to your other questions:




Is fire purely energy? Clearly not. The dancing flames are glowing gas--your suspicions confirmed.




Can fire be ionized? Is it affected by magnetism? Not so's you'd notice. You're thinking of plasma, which is ionized (and thus electromagnetically reactive) gas, often described as the fourth state of matter. You see it in welding arcs, lightning bolts, and the sun. Ordinary fire isn't plasma.











Is fire affected by gravity? Of course--gas has mass. Flame is shaped by convection, a function of gravity (hot air rises). In low- or zero-G environments, fire looks way different: a candle flame on the space shuttle isn't yellow and tapered but blue and nearly spherical.







 















So there you have it. One step closer to a better world.Rates and comments awaited....




 
Community shelf Community shelf -> Your name in Japanese -> Go to message
This Post 0 points    (Olaaa!! Perrrfect answer.   in 0 votes )   [?]
11 replies   
Mine is :
KASHIZUDOTO ZUKAKITU
Community shelf Community shelf -> What exactly is fire?is it pure energy? what state of matter is it? much more.... -> Go to message
This Post 0 points    (Olaaa!! Perrrfect answer.   in 0 votes )   [?]
1 replies   
Hey guys and gals please comment......
Community shelf Community shelf -> What exactly is fire?is it pure energy? what state of matter is it? much more.... -> Go to message
This Post 5 points    (Olaaa!! Perrrfect answer.   in 1 votes )   [?]
1 replies   

What exactly is fire? Is it purely energy? What state of matter is it? Can it be ionized? Can it be affected by magnetism? Gravity?


Confused,..well first think read the theory and then check for yourselves...


The correct definition needed to understand fire's properties is:


"Fire is the rapid combination of oxygen with fuel in the presence of heat, typically characterized by flame, a body of incandescent gas that contains and sustains the reaction and emits light and heat."




 






 




 





 


1) Rapid combination of oxygen with fuel in the presence of heat.Oxygen, fuel, and heat are the essential ingredients of fire. 




 


(2) Typically characterized by flame.  "Typically" allows mus to sidestep the issue of apparently nonflaming fires, like you get with burning charcoal. But charcoal fires do create flame--we just can't see it due to the lack of impurities or incompletely burned fuel in the plume. (we can't see a fuel fire at an Indy or CART race either, because the cars run on clean-burning methanol.) 


(3) Body of incandescent gas. Flame defined. Most encyclopedia and dictionary definitions blow past this entirely, allowing persons such as yourself to imagine that fire is "pure energy" or similar nonsense. We say "body" because the gas has a characteristic structure and composition. We say "incandescent" because (a) it sounds scientific, (b) it means "luminous with intense heat," precisely what we are attempting to convey. 


4) Contains and sustains the reaction. Flame isn't just the result of fire; it is the fire. What's more, without the flame's heat the fire would go out.


(5) Emits light and heat. Duh. However, we mustn't overlook the obvious.



 


Now to your other questions:




 


Is fire purely energy? Clearly not. The dancing flames are glowing gas--your suspicions confirmed.







                               


Can fire be ionized? Is it affected by magnetism? Not so's you'd notice. You're thinking of plasma, which is ionized (and thus electromagnetically reactive) gas, often described as the fourth state of matter. You see it in welding arcs, lightning bolts, and the sun. Ordinary fire isn't plasma.





Is fire affected by gravity? Of course--gas has mass. Flame is shaped by convection, a function of gravity (hot air rises). In low- or zero-G environments, fire looks way different: a candle flame on the space shuttle isn't yellow and tapered but blue and nearly spherical.







 





 

So there you have it. One step closer to a better world.Rates and comments awaited....

 
 
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